An improved light-cone harmonic oscillator model for the pionic leading-twist distribution amplitude
Abstract
In this paper, we study the pion leading-twist distribution amplitude φ2;π(x,μ) by improving the traditional light-cone harmonic oscillator model within the reconstruction of the function 2;π(x). In order to constraining the model parameters, we calculate its moments n2;π|μ in the framework of QCD background field theory sum rule (BFTSR) up to 10 th order. Considering the fact that the sum rule of the 0 th moment 02;π|μ cannot be normalized, we suggest a more reasonable sum rule formula for n2;π|μ. Then, we obtain the values of n2;π|μ0 with n=(2,4,6,8,10) at the initial scale μ0 = 1~ GeV. The first two moments are: 22;π|μ0 = 0.271 0.013, 42;π|μ0 = 0.138 0.010; and the corresponding Gegenbauer moments are a2;π2(μ0) = 0.206 0.038, a2;π4(μ0) = 0.047 0.011, respectively. After fitting the moments n2;π|μ, we obtained the appropriate model parameters by using the least square method. The resultant behavior for twist-2 pion DA is more closely to the AdS/QCD and lattice result, but is narrower than that by Dyson-Schwinger equation. Furthermore, we calculate the pion-photon transition form factors (TFF) and Bπ TFF within light-cone sum rule approach, which are conform with experimental and theoretical results.
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